Beta Apodis

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Template:Short description

Beta Apodis
Template:Location mark
Location of β Apodis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Apus
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) +4.24[2]
Characteristics
Evolutionary stage red clump[3]
Spectral type K0 III[4]
U−B Template:Engvar +0.95[2]
B−V Template:Engvar +1.06[2]
Astrometry
Radial velocity (Rv)−30.3±0.7[5] km/s
Proper motion (μ) RA: −281.986 mas/yr[1]
Dec.: −354.837 mas/yr[1]
Parallax (π)20.9535±0.1597 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)0.819[3]
Details
Mass1.84[3] Template:Solar mass
Radius11[6] Template:Solar radius
Luminosity50[6] Template:Solar luminosity
Surface gravity (log g)2.82±0.18[7] cgs
Temperature4,855±112[7] K
Metallicity [Fe/H]–0.03±0.04[7] dex
Rotational velocity (v sin i)1.3[8] km/s
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[9]
Database references
SIMBADdata

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Beta Apodis is a star in the southern circumpolar constellation of Apus. Its identifier is a Bayer designation that is Latinized from β Apodis, and abbreviated Bet Aps or β Aps, respectively. The apparent visual magnitude of this star is +4.24,[2] which is bright enough to be seen with the naked eye. It is located at a distance of approximately Script error: No such module "convert". from Earth,[1] as determined by parallax measurements. The star is drifting closer with a heliocentric radial velocity of −30 km/s.[5]

The spectrum of this star matches a stellar classification of K0 III,[4] which, according to models of stellar evolution, indicates that it is in the giant star stage, having exhausted the supply of hydrogen at its core. The measured angular diameter of this star is Script error: No such module "val"..[10] At the estimated distance of this star, this yields a physical size of about 11 times the radius of the Sun.[11] The expanded outer atmosphere of Beta Apodis has an effective temperature of about 4,855 K.[7] This heat is causing it to glow with the characteristic orange hue of a K-type star.[12]

Naming

In Chinese caused by adaptation of the European southern hemisphere constellations into the Chinese system, Script error: No such module "Lang". (Script error: No such module "Lang".), meaning Exotic Bird, refers to an asterism consisting of β Apodis, ζ Apodis, ι Apodis, γ Apodis, δ Octantis, δ1 Apodis, η Apodis, α Apodis and ε Apodis. Consequently, β Apodis itself is known as Script error: No such module "Lang". (Script error: No such module "Lang"., Template:Langx.)[13]

References

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  1. a b c d e Template:Cite Gaia EDR3
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  5. a b Script error: No such module "citation/CS1".
  6. a b Script error: No such module "citation/CS1".
  7. a b c d Script error: No such module "citation/CS1".
  8. Script error: No such module "citation/CS1".
  9. Template:Cite simbad
  10. Script error: No such module "citation/CS1".
  11. Script error: No such module "citation/CS1".. The radius (R*) is given by:
    2R*=(47.72.09103) AU0.0046491 AU/R22R
  12. Script error: No such module "citation/CS1".
  13. Template:In lang AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 29 日 Template:Webarchive

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External links

Template:Stars of Apus